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Ish: Shadow of rotating regular black holes
Generating rotating regular black hole solutions without complexification
MaqolaOchiq kirish201437 iqtibosABIGravitational lensing in a non-uniform plasma
G. S. Bisnovatyi-Kogan, O. Yu. Tsupko
MaqolaOchiq kirish201036 iqtibosABINon-Singular Charged Black Hole Solution for Non-Linear Source
Eloy Ayon-Beato, Alberto Garcia
MaqolaOchiq kirish199935 iqtibosABIOn gravitational lensing in the presence of a plasma
Oleg Yu. Tsupko, Г. С. Бисноватый-Коган
Maqola201234 iqtibosABIApparent shape of super-spinning black holes
Cosimo Bambi, Katherine Freese
MaqolaOchiq kirish200933 iqtibosABIShadows of Kerr Black Holes with Scalar Hair
Pedro V. P. Cunha, Carlos Herdeiro, Eugen Radu +1
MaqolaOchiq kirish201529 iqtibosABICircular geodesic of Bardeen and Ayon–Beato–Garcia regular black-hole and no-horizon spacetimes
MaqolaOchiq kirish201428 iqtibosABIThe apparent shape of a rotating charged black hole, closed photon orbits and the bifurcation set <i>A</i> <sub>4</sub>
MaqolaOchiq kirish199928 iqtibosABIConstraining the spin and the deformation parameters from the black hole shadow
Naoki Tsukamoto, Zilong Li, Cosimo Bambi
MaqolaOchiq kirish201420 iqtibosABIShapes and Positions of Black Hole Shadows in Accretion Disks and Spin Parameters of Black Holes
MaqolaOchiq kirish200418 iqtibosABIStrong Field Gravitational Lensing by a Kerr Black Hole
Samuel E. Vázquez, E. P. Esteban
Preprint200317 iqtibosABITESTING THE NO-HAIR THEOREM WITH OBSERVATIONS IN THE ELECTROMAGNETIC SPECTRUM. I. PROPERTIES OF A QUASI-KERR SPACETIME
Tim Johannsen, Dimitrios Psaltis
MaqolaOchiq kirish201017 iqtibosABIShape and position of the shadow in the δ = 2 Tomimatsu–Sato spacetime
MaqolaOchiq kirish201013 iqtibosABIAnalytic Kerr black hole lensing for equatorial observers in the strong deflection limit
V. Bozza, F. De Luca, G. Scarpetta +1
MaqolaOchiq kirish200512 iqtibosABIMeasuring the Kerr spin parameter of regular black holes from their shadow
MaqolaOchiq kirish201410 iqtibosABIQuasiequatorial gravitational lensing by spinning black holes in the strong field limit
MaqolaOchiq kirish200310 iqtibosABI